Exact(1)
Flow fields, residence time distribution, ozone concentration distribution, and concentration-contact time (CT) distribution within the contactor have been predicted via the computational framework.
Similar(7)
The impact of different stellar spectral energy distributions on the ozone distribution of habitable non-tidally locked terrestrial extrasolar planets has been studied by Selsis (2000), Segura et al.
Selsis et al. (2000), Segura et al. (2003), Segura et al. (2005), Grenfell et al. (2007), Rugheimer et al. (2013), Rauer et al. (2011) and Godolt et al. (2015) investigated the impact of different stellar spectral energy distributions on the ozone distribution of habitable non-tidally locked terrestrial extrasolar planets.
The results of such photochemical simulations gave trend in vertical distribution of ozone content.
It is therefore very important to consider the effect of solar proton events on the temporal and spatial distribution of ozone in the stratosphere.
Efforts to characterize spatial and temporal distribution of ozone (O3) in the 1999 Sierra Nevada study are compared with similar studies performed in North America and Europe.
Therefore, the vertical distribution of ozone VMR can be retrieved from the observed emission line shape by means of radiative transfer in a model atmosphere and an optimal estimation method.
It indicates that the score distribution of ozone has a remarkable overlap with that of ultrasound as their medians, lower percentiles, and upper percentiles are close to each other.
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Justyna Jupowicz-Kozak
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